Week 3 Flashcards

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1
Q

If you are looking at a wiggly line what is the wavelengths?

A

the difference in distance between the peaks

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2
Q

What is an example of a long and a short wavelength?

A

Long - radio/microwave - size of a building-butterfly

Short- Gamma ray or x-ray - size of atmoic nuclei-atoms

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3
Q

What is the colour relationship for long and short wavelengths?

A

Only a small visible range

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4
Q

What is the relationship between temperature and wavelength

A

cooler objects emit longer wavelenths, hotter objects emit shorter wavelengths

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5
Q

What kind of radiation can penetrate the earths atmosphere and what is in the grey and what can;t

A

CAN
Radio and infrared-visible

MAYBE
Some radio and some infrared

CANNOT
microwave and vible-gamaray short wave

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6
Q

What is Planck’s law

A

Hotter objects emit more radiation - higher specific spectral emittance

hotter objects emit short wave radiation and more radiation overall

the peak wavelength at which objects emit decreases with increasing temperature

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7
Q

What does the sun emit?

A

the peak is in the visible part of the spectrum

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8
Q

What kind of wavelength does the earth emit

A

the earth is colder the sun, emits in the infrared part of the spectrum

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9
Q

what percentage of the suns energy does the earth absorb and reflect?

A

70% absored
30% relected- espeically by light surfaces like clouds, snow and deserts

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10
Q

What is the unit of mesurement for radiative fluxes

A

W/m^2

the flow of energy through a given surface area over a certain amount of time

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11
Q

What is the global-mean incoming solar radiation and what is the net-absorbed solar radiation

A

global-mean incoming solar radaition = 340W/M^2

net-absorbed solar radiation is 240w/m^2

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12
Q

What is a radiative balance and how is it achieved?

A

energy in= energy out

emissions of infrared radiation to space

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13
Q

Without the atmosphere what temperature would the earth be?

A

-19oc

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14
Q

Without the ghg effect whast would the earth temperature be?

A

15oc

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15
Q

What is the Co2 content of the atmosphere for Earth and Venus?

A

.02% = earth
96% Venus

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16
Q

What is the ghg effect?

A

radiation emitted by earth is trapped by gases in the atmosphere and re-emitted in all directions

when it is re-emitted down this is the greenhouse effect

the large up and down longwave fluxes

idea that there is an asymmetry between absorption by ghg of infrared and visible radiation- traps infra-red

17
Q

What is albedo?

A

the reflection of solar energy depends on the albedo the earth atmosphere

high albedo - light reflective surfaces like snow and clouds
low albedo - dark surfaces like water and forests

18
Q

How do you calculate albedo?

A

albedo= reflected solar radiation/incoming solar radiation
1= everything is reflected 0= nothing is reflected

19
Q

What is the earths mean albedo

A

30%

however this varies spatially and depends on the surface type

20
Q

Where is shortwave radiation absorbed

A

mainly at the surface - some in the atmosphere but this is more UV rather than visible

Ozone layer - absorbs harmful carcogenic UV - holes in the ozone due to man-made CFCs

21
Q

Why are there different amounts of emission from different parts of the atmosphere

A

due to temperature changes - but what matters is the emissions out to space
typical level that escapes to space has a temperature that corresponds to that emission

22
Q

What is water vapour opque to?

A

infrared radiation at many wavelengths - therefore it absorbs it

23
Q

Why is there so much focus on carbon dioxide

A

it stays for longer in the atmosphere and thermodynamically unreative - very stable molecule once produced it will remain for a long time

24
Q

Methane from? and how much in the atmosphere?

A

gas leaks and livestock

has more than doubled

25
Q

Where is N2O from?

A

industrial processes, cars and fertilizers

26
Q

What does the absoption of radiation by ghg depend on?

A

the wavelength of infra red radiation

related to the molecular structure of the gases

27
Q

What is the water vapour window?

A

a range of wavelengths where eart is able to emit radiation to space.

Co2 is important as it partially masks the water vapour window - a range of wavelengths where the earth is able to emit to space

Increasing CO2 concentration partially close this window
- blocks more of the watervapour window

28
Q

What are sensible and latent heat fluxes?

A

Sensible heat is temperature - idea of a direct exchange of heat

Latent heat is humidity - like evaporation requires energy, condensation and then heating.

idea of fluxes by conduction and convection

29
Q

What does a postive imbalance mean for the earth?

A

the earth is absorbing more than it emits

the imbalance is mainly due to the strengthening of the greenhouse effect - though there are additional feedbacks

30
Q

What is radiative forcing?

A

an externally imposed instantaneous perturbation to the radiative balance - instantaneous perturbation

relative to some reference state it is measured by W/m^2

can be natural such as the sun’s orbit or human such as Co2
can be perturbing the energy in (solar radiation in) or energy out (how much escapes to space)

31
Q

Can you talk me through how GHG are a radative forcing?

A

Start in a radiative balance of the same amount of energy going in and out

increase in the amount of GHG means there is in>out - radiative forcing

the earth will accumulate heat thus warm

warming allows the earth to emit more radiative - Plancks Law

this continues until energy out is large enough - then a new equilibrium is reached

32
Q

Can you give some examples of forcings

A

Anthropogenic
- aerosol emissions - can reflect or absorb solar radiation
- land use change - surface albedo – contrails from airplanes

Natural
- solar activity variations
- volanic forcings - negative becausing of dimming aerosols -but these are v shortlived 2-3 yrs

33
Q

From the AR5 report what is the main forcing

A

Co2

methane and aerosol also have a substantial effect but large uncertainties around aerosols and clouds

34
Q

What is the effect of aerosols on the atmosphere?

A

Most have a cooling effectas they directly reflect sunlight or promote the formation of white clouds

however, black carbon has a warming effect as it absorbs sunlight in the atmosphere

there are large regional and temporal differences in aerosol production due to patterns of industry

they don’t mix well in the atmosphere so are quite localised in their effect

35
Q

If there is suddenly a doubling of the CO2 what would the temperature response look like on a graph?

what about the radiative imbalance line?

A

Temp
It would be flat until the forcing point then gradually and in a curve warm - and then stablise - initially fsater and then increasingly slowly as it plateus

exponential to begin with then decay to equilibrium

Radiative balance
- sharp increase at forcing point and then a gradual decline to equilibrium
proportional to the temperature change

Plancks law. idea that there is a relationship between temp and wavelength and the net energy emissions -as temperature increases earth radiates more energy and decreases the energy imbalance

36
Q

what is the energy budget equation ?

A

Radiative Imbalance = N

Radiative forcing = F (initial forcing)

Radiative response = § (or teepee, trainge T)

N= F-§

37
Q

What happens if F>0

A

the earth needs to warm in order to emit more infrared energy to space and re-establish a balance and vice versa (F<0 is a cooling)

38
Q

Would a postive forcing cool or warm

A

warming